Determination of nonuniversal supergravity models at the Large Hadron Collider

被引:12
作者
Dutta, Bhaskar [1 ]
Kamon, Teruki [1 ,2 ,3 ]
Krislock, Abram [1 ]
Kolev, Nikolay [4 ]
Oh, Youngdo [3 ]
机构
[1] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
[2] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[3] Kyungpook Natl Univ, Dept Phys, Taegu 702701, South Korea
[4] Univ Regina, Dept Phys, Regina, SK S4S 0A2, Canada
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 11期
关键词
NEUTRALINO-STAU COANNIHILATION; SUPERSYMMETRIC DARK-MATTER; MINIMAL SUPERGRAVITY; RELIC DENSITY; PARAMETER SPACE; MSSM; MASS; REGION; UNIFICATION; SIGNALS;
D O I
10.1103/PhysRevD.82.115009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine a well-motivated nonuniversal supergravity model where the Higgs boson masses are not unified with the other scalars at the grand unified scale at the LHC. The dark matter content can easily be satisfied in this model by having a larger Higgsino component in the lightest neutralino. Typical final states in such a scenario at the LHC involve W bosons. We develop a bi-event subtraction technique to reduce a huge combinatorial background to identify W -> jj decays. This is also a key technique to reconstruct supersymmetric particle masses in order to determine the model parameters. With the model parameters, we find that the dark matter content of the Universe can be determined in agreement with existing experimental results.
引用
收藏
页数:11
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